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G. Shaifullah

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Preprint Oct 2026

Modeling the nanohertz gravitational wave background with the t-process: Improved frequentist analysis of gravitational-wave power

Pulsar timing array (PTA) collaborations have recently reported evidence for a gravitational wave background (GWB) signal in the nanohertz band, which most likely originates from the incoherent superposition of GWs emitted by a population of supermassive black hole binaries (SMBHBs). Since the number of binaries emitti...

B. E. Moreschi, K. Gersbach, G. Shaifullah et al. · 0 citations

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